Fig. B.5
Halo WDLFs based on the assumption that all halo WDs originate from ZAMS stars in a single bin of the age-metallicity map (Fig. B.1). Colours for age and metallicity values are the same as in Figs. B.1, B.2, and B.4. The yellow lines with errorbars show the observed halo WDLF derived from selected halo WDs in the SuperCOSMOS Sky Survey (Rowell & Hambly 2011).
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